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pro vyhledávání: '"Casey, Andy"'
Autor:
Clark, Jake T., Clerte, Mathieu, Hinkel, Natalie R., Unterborn, Cayman T., Wittenmyer, Robert A., Horner, Jonathan, Wright, Duncan J., Carter, Brad, Morton, Timothy D., Spina, Lorenzo, Asplund, Martin, Buder, Sven, Bland-Hawthorn, Joss, Casey, Andy, De Silva, Gayandhi, D'Orazi, Valentina, Duong, Ly, Hayden, Michael, Freeman, Ken, Kos, Janez, Lewis, Geraint, Lin, Jane, Lind, Karin, Martell, Sarah, Sharma, Sanjib, Simpson, Jeffrey, Zucker, Dan, Zwitter, Tomaz, Tinney, Christopher G., Ting, Yuan-Sen, Nordlander, Thomas, Amarsi, Anish M.
An unprecedented number of exoplanets are being discovered by the Transiting Exoplanet Survey Satellite (TESS). Determining the orbital parameters of these exoplanets, and especially their mass and radius, will depend heavily upon the measured physic
Externí odkaz:
http://arxiv.org/abs/2008.05372
Autor:
Franchini, Mariagrazia, Morossi, Carlo, Di Marcantonio, Paolo, Chavez, Miguel, Gilmore, Gerry, Randich, Sofia, Flaccomio, Ettore, Koposov, Sergey E., Korn, Andreas J., Bayo, Amelia, Carraro, Giovanni, Casey, Andy, Franciosini, Elena, Hourihane, Anna, Jofre`, Paula, Lardo, Carmela, Lewis, James, Magrini, Laura, Morbidelli, Lorenzo, Sacco, G. G., Worley, Clare, Zwitter, Tomaz
We present a high resolution synthetic spectral library, INTRIGOSS, designed for studying FGK stars. The library is based on atmosphere models computed with specified individual element abundances via ATLAS12 code. Normalized SPectra (NSP) and surfac
Externí odkaz:
http://arxiv.org/abs/1806.08096
Autor:
Nordlander, Thomas, Amarsi, Anish M., Lind, Karin, Asplund, Martin, Barklem, Paul S., Casey, Andy R., Collet, Remo, Leenaarts, Jorrit
Publikováno v:
A&A 597, A6 (2017)
Models of star formation in the early universe depend on the details of accretion, fragmentation and radiative feedback. Different simulations predict different initial mass functions of the first stars, ranging from predominantly low mass (0.1-10 Ms
Externí odkaz:
http://arxiv.org/abs/1609.07416
Autor:
Hislop, Lachlan, Mould, Jeremy, Schmidt, Brian, Bessell, Michael S., Da Costa, Gary, Francis, Paul, Keller, Stefan, Tisserand, Patrick, Rapoport, Sharon, Casey, Andy
The Cepheid period-luminosity relation is the primary distance indicator used in most determinations of the Hubble constant. The tip of the red giant branch (TRGB) is an alternative basis. Using the new ANU SkyMapper Telescope, we calibrate the Tully
Externí odkaz:
http://arxiv.org/abs/1104.0974
Akademický článek
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